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| Yazar: | |
|---|---|
| Materyal Türü: | Recurso digital |
| Dil: | İngilizce |
| Baskı/Yayın Bilgisi: |
Zenodo
2026
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| Konular: | |
| Online Erişim: | https://doi.org/10.5281/zenodo.19096233 |
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İçindekiler:
- <h2>Abstract</h2> <p>This dataset presents the complete observational analysis supporting Chapter 10 of the monograph <strong>"Ontotopology of the Field: A Manifesto of Dynamic Connectivity"</strong> (Glushkov, 2026). The Ontopole theory proposes that the universe is a single continuous energy field Φ(x,n) with viscosity η_field, and that gravitational effects traditionally attributed to dark matter arise from local variations in field viscosity.</p> <p>We introduce the <strong>Cluster Viscosity Index (CVI)</strong> as a quantitative proxy for local field viscosity:</p> <p><span><span><span>CVI=(σv2Rcore)⋅(LxMbar)</span><span><span><span><span>CVI</span></span><span>=</span></span><span><span><span><span>(</span></span><span><span><span><span><span><span>R</span><span><span><span><span>core</span></span></span><span></span></span><span>σ</span><span><span><span>v</span></span><span><span>2</span></span><span></span></span></span><span></span></span></span></span></span><span><span>)</span></span></span><span>⋅</span></span><span><span><span><span>(</span></span><span><span><span><span><span><span>M</span><span><span><span><span>bar</span></span></span><span></span></span><span>L</span><span><span><span>x</span></span><span></span></span></span><span></span></span></span></span></span><span><span>)</span></span></span></span></span></span></span></p> <p>where σ_v is velocity dispersion, R_core is core radius, L_x is X-ray luminosity, and M_bar is baryonic mass.</p> <p>Eight massive galaxy clusters with well-documented gravitational lensing anomalies are analyzed:</p> <ol> <li> <p><strong>Abell 2744</strong> (Pandora's Cluster) — z = 0.308, merger of four clusters</p> </li> <li> <p><strong>MACS J0717.5+3745</strong> — z = 0.546, largest known gravitational lens, 18 Mpc filament</p> </li> <li> <p><strong>Abell 1689</strong> — z = 0.183, anomalously steep mass profile</p> </li> <li> <p><strong>Abell 520</strong> — z = 0.200, "dark core" without galaxies, line-of-sight filament</p> </li> <li> <p><strong>MACS J0025.4-1222</strong> — z = 0.586, "Bullet Twin," two equal subclusters</p> </li> <li> <p><strong>1E 0657-56</strong> (Bullet Cluster) — z = 0.296, classic merger</p> </li> <li> <p><strong>ClG J1226.9+3332</strong> — z = 0.892, high redshift</p> </li> <li> <p><strong>MACS J0416.1-2403</strong> — z = 0.396, complex double structure</p> </li> </ol> <h3>Key Results</h3> <ul> <li> <p><strong>Correlation confirmed</strong>: Clusters with higher CVI show systematic lensing anomalies, with a Pearson correlation coefficient r = 0.28.</p> </li> <li> <p><strong>Four dynamical regimes identified</strong> corresponding to different types of field-vortex interactions:</p> <ul> <li> <p>Regime I (CVI 1-3 × 10³⁴): Moderate turbulence, M_total/M_bar = 5-10</p> </li> <li> <p>Regime II (CVI 4-5 × 10³⁴): Extreme turbulence, M_total/M_bar = 4-5</p> </li> <li> <p>Regime III (CVI 8-10 × 10³⁴): Directed collision, M_total/M_bar = 6-7</p> </li> <li> <p>Regime IV (CVI >10 × 10³⁴): Anomalous concentration, M_total/M_bar ≈ 4.7</p> </li> </ul> </li> <li> <p><strong>Geometric effects critical</strong>: Abell 520 shows high anomaly (5.9) at moderate CVI (2.02) due to line-of-sight filament projection.</p> </li> <li> <p><strong>Extreme turbulence reduces anomaly</strong>: Abell 2744 with maximum CVI (4.83) shows minimum anomaly (4.0) due to energy dissipation through eight substructures.</p> </li> <li> <p><strong>Redshift independence</strong>: Clusters from z = 0.2 to z = 0.9 show consistent behavior, confirming local field dynamics dominance.</p> </li> <li> <p><strong>Direct filament observation</strong>: MACS J0717.5+3745's 18 Mpc filament provides direct evidence of field viscosity gradients at megascales.</p> </li> </ul> <h3>Conclusion</h3> <p>The observed gravitational lensing anomalies in all eight clusters can be explained within the Ontopole framework without invoking hypothetical dark matter particles. The effects arise as consequences of local field viscosity increase η_local in regions of intense vortex dynamics. This analysis provides the first quantitative observational test of the Ontopole field theory.</p> <h3>Dataset Contents</h3> <ul> <li> <p>Complete dataset in CSV format with all cluster parameters and uncertainties</p> </li> <li> <p>Python scripts for CVI calculation and visualization</p> </li> <li> <p>High-resolution figures including correlation plots</p> </li> <li> <p>Full preprint of Chapter 10 with detailed analysis</p> </li> <li> <p>Comprehensive bibliography with 40+ references</p> </li> </ul> <h3>DOI</h3> <p><strong>10.5281/zenodo.19096233</strong></p>